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Extending the supernova Hubble diagram to z similar to 1.5 with the Euclid space mission

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Extending the supernova Hubble diagram to z similar to 1.5 with the Euclid space mission. / Astier, P.; Balland, C.; Brescia, M. et al.
In: Astronomy and Astrophysics, Vol. 572, 80, 12.2014.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Astier, P, Balland, C, Brescia, M, Cappellaro, E, Carlberg, RG, Cavuoti, S, Della Valle, M, Gangler, E, Goobar, A, Guy, J, Hardin, D, Hook, IM, Kessler, R, Kim, A, Linder, E, Longo, G, Maguire, K, Mannucci, F, Mattila, S, Nichol, R, Pain, R, Regnault, N, Spiro, S, Sullivan, M, Tao, C, Turatto, M, Wang, XF & Wood-Vasey, WM 2014, 'Extending the supernova Hubble diagram to z similar to 1.5 with the Euclid space mission', Astronomy and Astrophysics, vol. 572, 80. https://doi.org/10.1051/0004-6361/201423551

APA

Astier, P., Balland, C., Brescia, M., Cappellaro, E., Carlberg, R. G., Cavuoti, S., Della Valle, M., Gangler, E., Goobar, A., Guy, J., Hardin, D., Hook, I. M., Kessler, R., Kim, A., Linder, E., Longo, G., Maguire, K., Mannucci, F., Mattila, S., ... Wood-Vasey, W. M. (2014). Extending the supernova Hubble diagram to z similar to 1.5 with the Euclid space mission. Astronomy and Astrophysics, 572, Article 80. https://doi.org/10.1051/0004-6361/201423551

Vancouver

Astier P, Balland C, Brescia M, Cappellaro E, Carlberg RG, Cavuoti S et al. Extending the supernova Hubble diagram to z similar to 1.5 with the Euclid space mission. Astronomy and Astrophysics. 2014 Dec;572:80. Epub 2014 Dec 1. doi: 10.1051/0004-6361/201423551

Author

Astier, P. ; Balland, C. ; Brescia, M. et al. / Extending the supernova Hubble diagram to z similar to 1.5 with the Euclid space mission. In: Astronomy and Astrophysics. 2014 ; Vol. 572.

Bibtex

@article{66f71353429247bd92f5e6e826e238e8,
title = "Extending the supernova Hubble diagram to z similar to 1.5 with the Euclid space mission",
abstract = "We forecast dark energy constraints that could be obtained from a new large sample of Type Ia supernovae where those at high redshift are acquired with the Euclid space mission. We simulate a three-prong SN survey: a z <0.35 nearby sample (8000 SNe), a 0.2 ",
keywords = "cosmological parameters, dark energy, ACTIVE GALACTIC NUCLEI, CORE-COLLAPSE SUPERNOVAE, DELAY-TIME DISTRIBUTION, PHOTOMETRY DATA RELEASE, HOST GALAXY PROPERTIES, STAR-FORMATION RATE, DARK ENERGY SURVEY, II-P SUPERNOVAE, IA LIGHT CURVES, LEGACY SURVEY",
author = "P. Astier and C. Balland and M. Brescia and E. Cappellaro and Carlberg, {R. G.} and S. Cavuoti and {Della Valle}, M. and E. Gangler and A. Goobar and J. Guy and D. Hardin and Hook, {I. M.} and R. Kessler and A. Kim and E. Linder and G. Longo and K. Maguire and F. Mannucci and S. Mattila and R. Nichol and R. Pain and N. Regnault and S. Spiro and M. Sullivan and C. Tao and M. Turatto and Wang, {X. F.} and Wood-Vasey, {W. M.}",
year = "2014",
month = dec,
doi = "10.1051/0004-6361/201423551",
language = "English",
volume = "572",
journal = "Astronomy and Astrophysics",
issn = "0004-6361",
publisher = "EDP Sciences",

}

RIS

TY - JOUR

T1 - Extending the supernova Hubble diagram to z similar to 1.5 with the Euclid space mission

AU - Astier, P.

AU - Balland, C.

AU - Brescia, M.

AU - Cappellaro, E.

AU - Carlberg, R. G.

AU - Cavuoti, S.

AU - Della Valle, M.

AU - Gangler, E.

AU - Goobar, A.

AU - Guy, J.

AU - Hardin, D.

AU - Hook, I. M.

AU - Kessler, R.

AU - Kim, A.

AU - Linder, E.

AU - Longo, G.

AU - Maguire, K.

AU - Mannucci, F.

AU - Mattila, S.

AU - Nichol, R.

AU - Pain, R.

AU - Regnault, N.

AU - Spiro, S.

AU - Sullivan, M.

AU - Tao, C.

AU - Turatto, M.

AU - Wang, X. F.

AU - Wood-Vasey, W. M.

PY - 2014/12

Y1 - 2014/12

N2 - We forecast dark energy constraints that could be obtained from a new large sample of Type Ia supernovae where those at high redshift are acquired with the Euclid space mission. We simulate a three-prong SN survey: a z <0.35 nearby sample (8000 SNe), a 0.2

AB - We forecast dark energy constraints that could be obtained from a new large sample of Type Ia supernovae where those at high redshift are acquired with the Euclid space mission. We simulate a three-prong SN survey: a z <0.35 nearby sample (8000 SNe), a 0.2

KW - cosmological parameters

KW - dark energy

KW - ACTIVE GALACTIC NUCLEI

KW - CORE-COLLAPSE SUPERNOVAE

KW - DELAY-TIME DISTRIBUTION

KW - PHOTOMETRY DATA RELEASE

KW - HOST GALAXY PROPERTIES

KW - STAR-FORMATION RATE

KW - DARK ENERGY SURVEY

KW - II-P SUPERNOVAE

KW - IA LIGHT CURVES

KW - LEGACY SURVEY

U2 - 10.1051/0004-6361/201423551

DO - 10.1051/0004-6361/201423551

M3 - Journal article

VL - 572

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

SN - 0004-6361

M1 - 80

ER -